Plasmoid Instability in Forming Current Sheets

The plasmoid instability has revolutionized our understanding of magnetic reconnection in astrophysical environments. By preventing the formation of highly elongated reconnection layers, it is crucial in enabling the rapid energy conversion rates that are characteristic of many astrophysical phenome...

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Veröffentlicht in:	The Astrophysical journal 2017-12, Vol.850 (2), p.142
Hauptverfasser:	Comisso, L., Lingam, M., Huang, Y.-M., Bhattacharjee, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aspect ratio ASTRONOMY AND ASTROPHYSICS Astrophysics Corona Current sheets Energy conversion Growth rate Instability Interstellar matter Interstellar medium ISM: magnetic fields Linear phase Magnetic reconnection magnetohydrodynamics plasmas Prandtl number Scaling laws Solar corona Stability stars: coronae Sun: flares Wavelengths
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